According to the actual volume of gas molecule and effort between molecules influencing the gas action, in the Van der Waal formula of ideal gas state, the amending terms of n~2a/v~2 and nb is introduced and then the formula (p+n~2a/v~2)(v-nb)=nRT forms to describe the actual gas action.
范德华针对实际气体分子自身体积和分子间作用力对气体行为的影响,在理想气体状态方程式中引入修正项n2aV2)(V-nb)=V2和nb而得出描述实际气体行为的方程式———范德华方程式(P+n2anRT。
This article discusses actual gas by means of statistical thermodynamics and draws two conclusions:(1)In actual application there will be some gas which meets pV=nRT relatively,but don t meet U=(T).
本文用统计热力学的方法讨论了实际气体,指出:在实际应用中会出现在某些条件下满足pV=nRT但不满足U=(T);绝对满足理想气体状态方程的气体一定满足焦耳定律。
A new method is presented to calculate temperature extremum of actual gas in arbitrary process and an example is given.
给出了一种普遍求解实际气体经过任意过程温度极值的计算方法,并举例进行了讨论。
Another method for resolving internal energy of real gases;
实际气体内能的另一求法
A study on the process of quasi-static state of real gas;
实际气体准静态过程的研究
In the paper, modification suggestion to Vander Waals gas model is provided;state equation and internal energy formula which are more suitable for characteristic of real gas are derived.
该文对范德瓦尔斯气体模型提出修改意见,并导出更符合实际气体特点的状态方程和内能公式。
Three dimensional turbulent R134a gas flow in an unshrouded centrifugal compressor impeller is numerically simulated using real gas model.
使用实际气体模型对R134a在半开式离心压缩机叶轮内部三维湍流进行了数值计算,比较了比容比相等情况下实际及理想气体模型对压缩过程的差异。
These elements become part of the interstellar gas and dust.
这些元素成了星际气体和星际尘埃的一部分。
We will be interested in the heat capacity of interstellar gases.
我们感兴趣的是星际气体的热容量。
The magnetic lines of force are in effect glued to the interstellar gas, and they follow the clouds in their capricious motions.
磁力线实际上是紧附在星际气体上，并跟随星际云一道作着变化莫测的运动。
These tiny regions may be condensations in the interstellar gas where stars and planetary systems could be forming.
这些很小的区域可能是能够形成恒星或行星系统的星际气体中的一些凝聚体。
Interstellar gas clouds frequently collide and convert their kinetic energy into shock waves and radiation.
星际气体云经常在碰撞间将动能传给冲击波和辐射。
The concentrations of interstellar gas can now be mapped with much great accuracy than would ever be possible using visible light.
如今，可以画出比用可见光更精确的星际气体聚集图。
The contraction of a cool interstellar gas cloud can proceed in a variety of ways.
一个冷的星际气体云的收缩，可以通过许多不同的方式来进行。
Our assertion that the interstellar gas is definitely no vacuum would seem all the more paradoxical!
我们坚持星际气体决非真空的主张看来愈发荒谬可笑了！
The remnant nebular gas pervades the interplanetary space.
星云的残余气体充斥星际空间。
clouds of particles or gases occurring throughout interstellar space.
遍及星际空间的微粒或气体组成的云。
Such tumultuous, often visually spectacular, interstellar regions surrounding youthful stars are known as gaseous nebulae.
这种环绕着年轻星的动荡且常常是壮观的星际区域，叫做气体星云。
A star is formed when a cloud of gas collapses from the interstellar medium toward high density.
一个气体云自星际物质中坍缩，密度达到很高时，即形成了一个恒星。
International Satellite Cloud Climatology Project
国际卫星云气候学项目
International Satellite Cloud Climatology Project (ISCCP)
国际卫星云气候学计划
International Polar Orbiting Meteorological Satellite
国际极轨道气象卫星
The solar wind does not impinge directly on the earth and its atmosphere, however.
太阳风一直向外吹，直到碰到星际中的离子或电中性气体。
an immense cloud of gas (mainly hydrogen) and dust in interstellar space.
在星际空间中的一种无边的由气体（主要成分为氢）和灰尘组成的云。
We consider the macroscopic thermal properties of the gas throughout the interstellas region ionized by an exciting star or group of stars.
我们将考察被一颗或一群激发星电离的星际区域中各种气体的宏观热力学性质。